With growing data volumes from synoptic surveys, astronomers necessarily must become more abstracted from the discovery and introspection processes. Given the scarcity of follow-up resources, there is a particularly sharp onus on the frameworks that replace these human roles to provide accurate and well-calibrated probabilistic classification catalogs. Such catalogs inform the subse-quent follow-up, allowing consumers to optimize the selection of specific sources for further study and permitting rigorous treatment of purities and efficiencies for population studies. Here, we describe a process to produce a probabilistic classification catalog of variability with machine learning from a multi-epoch pho-tometric survey. In addition to produci...
We used 3.1 million spectroscopically labelled sources from the Sloan Digital Sky Survey (SDSS) to t...
This is version 1, you should use the updated version 2 that was accepted for publication: 10.5281/z...
This is the same as the published data available under 10.5281/zenodo.3768398, but in the format of ...
We consider the statistical problem of catalogue matching from a machine learning perspective with t...
Advances in the development of detector and computer technology have led to a rapid increase in the ...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
Modern time-domain surveys continuously monitor large swaths of the sky to look for astronomical var...
Cataloging is an essential part of the data processing pipelines of modern surveys: most astrophysic...
Context. In current astronomical surveys with ever-increasing data volumes, automated methods are es...
Context. In current astronomical surveys with ever-increasing data volumes, automated methods are es...
The Paper: https://arxiv.org/abs/1909.10963 Abstract: We used 3.1 million spectroscopically labelle...
We consider the statistical problem of catalogue matching from a machine learning perspective with t...
In this paper we address two questions related to data analysis in large astronomical datasets, and ...
We used 3.1 million spectroscopically labelled sources from the Sloan Digital Sky Survey (SDSS) to t...
This is version 1, you should use the updated version 2 that was accepted for publication: 10.5281/z...
This is the same as the published data available under 10.5281/zenodo.3768398, but in the format of ...
We consider the statistical problem of catalogue matching from a machine learning perspective with t...
Advances in the development of detector and computer technology have led to a rapid increase in the ...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
There is an increasing number of large, digital, synoptic sky surveys, in which repeated observation...
Modern time-domain surveys continuously monitor large swaths of the sky to look for astronomical var...
Cataloging is an essential part of the data processing pipelines of modern surveys: most astrophysic...
Context. In current astronomical surveys with ever-increasing data volumes, automated methods are es...
Context. In current astronomical surveys with ever-increasing data volumes, automated methods are es...
The Paper: https://arxiv.org/abs/1909.10963 Abstract: We used 3.1 million spectroscopically labelle...
We consider the statistical problem of catalogue matching from a machine learning perspective with t...
In this paper we address two questions related to data analysis in large astronomical datasets, and ...
We used 3.1 million spectroscopically labelled sources from the Sloan Digital Sky Survey (SDSS) to t...
This is version 1, you should use the updated version 2 that was accepted for publication: 10.5281/z...
This is the same as the published data available under 10.5281/zenodo.3768398, but in the format of ...